Sentinel-1 Detection of Ice Slabs on the Greenland Ice Sheet

Ice slabs are multi-meter-thick layers of refrozen ice that limit meltwater storage in firn, leading to enhanced surface runoff and ice sheet mass loss. To date, ice slabs have primarily been mapped using airborne ice-penetrating radar, which has limited spatial and temporal coverage. This makes it...

Full description

Bibliographic Details
Main Authors: Culberg, Riley, Michaelides, Roger J., Miller, Julie Z.
Format: Text
Language:English
Published: 2024
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2023-2652
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2652/
id ftcopernicus:oai:publications.copernicus.org:egusphere115896
record_format openpolar
spelling ftcopernicus:oai:publications.copernicus.org:egusphere115896 2024-06-23T07:53:14+00:00 Sentinel-1 Detection of Ice Slabs on the Greenland Ice Sheet Culberg, Riley Michaelides, Roger J. Miller, Julie Z. 2024-05-23 application/pdf https://doi.org/10.5194/egusphere-2023-2652 https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2652/ eng eng doi:10.5194/egusphere-2023-2652 https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2652/ eISSN: Text 2024 ftcopernicus https://doi.org/10.5194/egusphere-2023-2652 2024-06-13T01:23:50Z Ice slabs are multi-meter-thick layers of refrozen ice that limit meltwater storage in firn, leading to enhanced surface runoff and ice sheet mass loss. To date, ice slabs have primarily been mapped using airborne ice-penetrating radar, which has limited spatial and temporal coverage. This makes it difficult to fully assess the current extent and continuity of ice slabs or to validate predictive models of ice slab evolution that are key to understanding their impact on Greenland's surface mass balance. Here, for the first time, we map the extent of ice slabs and superimposed ice facies across the entire Greenland Ice Sheet at 500 m resolution using dual-polarization Sentinel-1 ( S-1 ) synthetic-aperture radar (SAR) data collected in winter 2016–2017. We do this by selecting empirical thresholds for the cross-polarized backscatter ratio and HV backscattered power that jointly optimize the agreement between airborne ice-penetrating radar data detections of ice slabs and the S-1 estimates of ice slab extent. Our results show that there is a strong correlation between C-band backscatter and the ice content of the upper ∼ 7 m of the firn column that enables ice slab mapping with S-1 . Our new mapping shows that ice slabs are nearly continuous around the entire margin of the ice sheet. This includes regions in southwest Greenland where ice slabs have not been previously identified by ice-penetrating radar but where the S-1 -inferred ice slab extent shows strong agreement with the extent of visible runoff mapped from optical imagery. The algorithm developed here lays the groundwork for the long-term monitoring of ice slab expansion with current and future C-band satellite systems and highlights the potential added value of future L-band missions for near-surface studies in Greenland. Text Greenland Ice Sheet Copernicus Publications: E-Journals Greenland
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Ice slabs are multi-meter-thick layers of refrozen ice that limit meltwater storage in firn, leading to enhanced surface runoff and ice sheet mass loss. To date, ice slabs have primarily been mapped using airborne ice-penetrating radar, which has limited spatial and temporal coverage. This makes it difficult to fully assess the current extent and continuity of ice slabs or to validate predictive models of ice slab evolution that are key to understanding their impact on Greenland's surface mass balance. Here, for the first time, we map the extent of ice slabs and superimposed ice facies across the entire Greenland Ice Sheet at 500 m resolution using dual-polarization Sentinel-1 ( S-1 ) synthetic-aperture radar (SAR) data collected in winter 2016–2017. We do this by selecting empirical thresholds for the cross-polarized backscatter ratio and HV backscattered power that jointly optimize the agreement between airborne ice-penetrating radar data detections of ice slabs and the S-1 estimates of ice slab extent. Our results show that there is a strong correlation between C-band backscatter and the ice content of the upper ∼ 7 m of the firn column that enables ice slab mapping with S-1 . Our new mapping shows that ice slabs are nearly continuous around the entire margin of the ice sheet. This includes regions in southwest Greenland where ice slabs have not been previously identified by ice-penetrating radar but where the S-1 -inferred ice slab extent shows strong agreement with the extent of visible runoff mapped from optical imagery. The algorithm developed here lays the groundwork for the long-term monitoring of ice slab expansion with current and future C-band satellite systems and highlights the potential added value of future L-band missions for near-surface studies in Greenland.
format Text
author Culberg, Riley
Michaelides, Roger J.
Miller, Julie Z.
spellingShingle Culberg, Riley
Michaelides, Roger J.
Miller, Julie Z.
Sentinel-1 Detection of Ice Slabs on the Greenland Ice Sheet
author_facet Culberg, Riley
Michaelides, Roger J.
Miller, Julie Z.
author_sort Culberg, Riley
title Sentinel-1 Detection of Ice Slabs on the Greenland Ice Sheet
title_short Sentinel-1 Detection of Ice Slabs on the Greenland Ice Sheet
title_full Sentinel-1 Detection of Ice Slabs on the Greenland Ice Sheet
title_fullStr Sentinel-1 Detection of Ice Slabs on the Greenland Ice Sheet
title_full_unstemmed Sentinel-1 Detection of Ice Slabs on the Greenland Ice Sheet
title_sort sentinel-1 detection of ice slabs on the greenland ice sheet
publishDate 2024
url https://doi.org/10.5194/egusphere-2023-2652
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2652/
geographic Greenland
geographic_facet Greenland
genre Greenland
Ice Sheet
genre_facet Greenland
Ice Sheet
op_source eISSN:
op_relation doi:10.5194/egusphere-2023-2652
https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2652/
op_doi https://doi.org/10.5194/egusphere-2023-2652
_version_ 1802644808189083648